New series of asymptotically flat axisymmetric and stationary gravitational solutions

Kyriakopoulos, E

dc.contributor.author	Kyriakopoulos, E	en
dc.date.accessioned	2014-03-01T01:07:12Z
dc.date.available	2014-03-01T01:07:12Z
dc.date.issued	1988	en
dc.identifier.issn	0001-7701	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/9854
dc.subject	General Relativity	en
dc.subject.classification	Astronomy & Astrophysics	en
dc.subject.classification	Physics, Multidisciplinary	en
dc.subject.classification	Physics, Particles & Fields	en
dc.title	New series of asymptotically flat axisymmetric and stationary gravitational solutions	en
heal.type	journalArticle	en
heal.identifier.primary	10.1007/BF00759027	en
heal.identifier.secondary	http://dx.doi.org/10.1007/BF00759027	en
heal.language	English	en
heal.publicationDate	1988	en
heal.abstract	The equations for the pseudopotential of Harrison's Bäcklund transformations with seed solution an asymptotically flat solution of the Ernst equation are solved. A new series of asymptotically flat solutions of the equations of general relativity is obtained from the determinants of matrices, whose elements are known. The first solution of the series is calculated as a ratio of two sums of monomials. This solution has five arbitrary real constants. For a particular choice of the constants it becomes Kerr's solution. © 1982 Plenum Publishing Corporation.	en
heal.publisher	Kluwer Academic Publishers-Plenum Publishers	en
heal.journalName	General Relativity and Gravitation	en
dc.identifier.doi	10.1007/BF00759027	en
dc.identifier.isi	ISI:A1988Q472500008	en
dc.identifier.volume	20	en
dc.identifier.issue	10	en
dc.identifier.spage	1067	en
dc.identifier.epage	1081	en